Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-08-14
Physics
High Energy Physics
High Energy Physics - Phenomenology
9 pages, 6 figs. Power spectrum movies at http://www.hep.upenn.edu/~max/concordance.html or from max@physics.upenn.edu. To a
Scientific paper
As experimentalists step up their pursuit of cold dark matter particles and neutrino masses, cosmological constraints are tightening. We compute the joint constraints on 11 cosmological parameters from cosmic microwave background and large scale structure data, and find that at 95% confidence, the total (cold+hot) dark matter density is h^2 Omega_dark = 0.20 +.12 -.10 with at most 38% of it being hot (due to neutrinos). A few assumptions, including negligible neutrinos, tighten this measurement to h^2 Omega_dark = 0.13 +0.04 -0.02, i.e, 2.4e-27 kg/m^3 give or take 20%.
Hamilton Andrew J. S.
Tegmark Max
Zaldarriaga Matias
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